Photometry of Nova Cygni '78 /V 1668 Cyg/ - Evidence for a post-maximum short time periodicity

Details Photometry of Nova Cygni '78 /V 1668 Cyg/ - Evidence for a post-maximum short time periodicity Photometry of Nova Cygni '78 /V 1668 Cyg/ - Evidence for a post-maximum short time periodicity

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85l...4c&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 1-2, May 1980, p. L4, L5.

Astronomy and Astrophysics

Astrophysics

7

Astronomical Photometry, Binary Stars, Novae, Electrophotometers, Light Curve, Periodic Variations

Scientific paper

Photoeleotrical measurements of Nova Cygni '78 show short period
oscillations superposed on the secular decrease. The period is
10h.54 and the amplitude 0m.15; these
peculiarities are close to those detected in the Nova Cyg '75 light
curve.

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